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The mass distribution of the first stars can be determined via the 21-cm signal (2025)

First Author: Gessey-Jones T
Attributed to:  Planet Formation in Binary Stars funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2502.18098

Publication URI: https://arxiv.org/abs/2502.18098

Type: Preprint